Exploring the links between quasar winds and radio emission along the main sequence at high redshift

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Table 5.

Measurements on the Hβ full broad line profile and derived properties of the Hβ region.

Source	F_5100 Å	F_tot	W	FWHM	A.I.	c(1/4)	c(1/2)	c(3/4)	c(9/10)	R_Fe II	ST	log L_bol	log M_BH	log L/L_Edd
			[Å]	[km s⁻¹]		[km s⁻¹]	[km s⁻¹]	[km s⁻¹]	[km s⁻¹]			[erg s⁻¹]	[M_⊙]
(1)	(2)	(3)	(4)	(5)	(6)	(7)	(8)	(9)	(10)	(11)	(12)	(13)	(14)	(15)
Population A

BZQJ0544-2241	4.53	2.52	51	5191 ± 458	−0.05 ± 0.09	−266 ± 402	−174 ± 93	−94 ± 141	−57 ± 170	0.69	A2	47.52	9.66	−0.31
WB J0948+0855 ^(a)	2.88	1.27	43	5580 ± 494	0.00 ± 0.11	−1 ± 456	−1 ± 92	0 ± 149	0 ± 184	0.89	A2	47.45	9.74	−0.46
CTSJ01.03	1.96	1.73	81	4551 ± 403	0.00 ± 0.20	320 ± 372	321 ± 75	321 ± 122	321 ± 150	0.21	A1	47.37	9.52	−0.33
FBQS J2149-0811	1.73	1.80	113	4992 ± 442	0.00 ± 0.11	0 ± 408	0 ± 82	−1 ± 133	−1 ± 165	0.23	A1	47.26	9.55	−0.46

Population B

PKS0226-038	1.48	0.99	66	5280 ± 420	0.46 ± 0.05	2874 ± 646	109 ± 53	−45 ± 140	−86 ± 190	0.62	B2	47.18	9.44	−0.44
PKS0237-23	5.19	4.48	89	7986 ± 821	0.31 ± 0.11	2546 ± 389	1374 ± 65	730 ± 211	574 ± 262	0.42	B1	47.76	9.85	−0.27
PKS0858-279 ^(a)	12.9	7.84	56	5385 ± 402	0.15 ± 0.11	790 ± 388	299 ± 61	191 ± 141	159 ± 191	0.47	B1	48.14	9.91	0.05
CTSJ03.14 ^(a)	3.44	3.61	102	4056 ± 305	0.07 ± 0.09	271 ± 274	100 ± 52	62 ± 106	50 ± 143	0.38	B1	47.62	9.36	0.08
PKS1448-232	3.43	4.53	129	4397 ± 364	0.54 ± 0.09	3664 ± 745	263 ± 47	150 ± 114	122 ± 153	0.07	B1	47.58	9.43	−0.02
[HB89]1559+088	3.31	3.66	110	5802 ± 514	0.01 ± 0.18	71 ± 750	−314 ± 115	−39 ± 157	13 ± 184	0.29	B1	47.57	9.56	−0.16

Notes. (1) Source identification. (2) Flux of the continuum on the 5100 Å wavelength, corrected for galactic extinction, in units of 10⁻¹⁵ erg s⁻¹ cm⁻² Å⁻¹. (3) Full Hβ line flux (i.e., the flux for all broad line components, BC, and VBC, and BLUE whenever appropriate), in units of 10⁻¹³ erg s⁻¹ cm⁻². (4) Hβ equivalent width W. (5) FWHM. (6) Asymmetry index (A.I.). (7), (8), (9), (10) Centroid velocity shifts at $\frac{1}{4}$ $\frac{1}{4}$ , $\frac{1}{2}$ $\frac{1}{2}$ , $\frac{3}{4}$ $\frac{3}{4}$ , and $\frac{9}{10}$ $\frac{9}{10}$ fractional intensities. (11) Ratio R_Fe II (see Sect. 4.2). (12) Spectral types according to the quasar main sequence. (13) Bolometric luminosity. (14) Black hole mass. (15) Eddington ratio.

^(a)

Hβ profile may be affected by the correction of the telluric absorptions present in the spectrum (see Zenodo).

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